The NeXT Mission
T. Takahashi, R.Kelley, K. Mitsuda, H. Kunieda, R. Petre, N. White, T., Dotani, R. Fujimoto, Y. Fukazawa, K. Hayashida, M. Ishida, Y. Ishisaki, M., Kokubun, K. Makishima, K. Koyama, G.M. Madejski, K. Mori, R. Mushotzky, K., Nakazawa, Y. Ogasaka, T. Ohashi, M. Ozaki, H. Tajima

TL;DR
The NeXT mission is an international X-ray observatory designed to explore a broad energy range from soft X-rays to soft gamma-rays with high spectral resolution, enabling advanced astrophysical research.
Contribution
It introduces a novel combination of wide-band X-ray instruments, including focusing mirrors, micro-calorimeters, and gamma-ray detectors, for comprehensive high-resolution X-ray astronomy.
Findings
Wide energy coverage from 0.3 keV to 600 keV.
High spectral resolution micro-calorimeter with Delta E ~ 7 eV.
International collaboration for advanced X-ray instrumentation.
Abstract
The NeXT (New exploration X-ray Telescope), the new Japanese X-ray Astronomy Satellite following Suzaku, is an international X-ray mission which is currently planed for launch in 2013. NeXT is a combination of wide band X-ray spectroscopy (3 - 80 keV) provided by multi-layer coating, focusing hard X-ray mirrors and hard X-ray imaging detectors, and high energy-resolution soft X-ray spectroscopy (0.3 - 10 keV) provided by thin-foil X-ray optics and a micro-calorimeter array. The mission will also carry an X-ray CCD camera as a focal plane detector for a soft X-ray telescope and a non-focusing soft gamma-ray detector. With these instruments, NeXT covers very wide energy range from 0.3 keV to 600 keV. The micro-calorimeter system will be developed by international collaboration lead by ISAS/JAXA and NASA. The simultaneous broad bandpass, coupled with high spectral resolution of Delta E ~ 7…
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